Barnard's Star d

Planet· orbits Barnard's Star

Barnard's Star d — the innermost and hottest of the four (equilibrium temperature ~480 K), a sub-Earth on a 2.34-day orbit. Never imaged; appearance unknown.

Open in 3D viewSee Barnard's Star d in the live, interactive 3D map

Key facts

Minimum mass
1.57 × 10²⁴ kg
0.263 M⊕
Year
2.34 Earth days
Distance from Barnard's Star
2,812,440 km

Science

Physical

Minimum mass (m·sin i)
1.57 × 10²⁴ kg · 0.263 M⊕
Radial-velocity detection measures m·sin i; the true mass depends on the unknown orbital inclination.
Radius
Not measured
No transit — radius is a model estimate; true size unknown.

Orbital

Semi-major axis
2,812,440 km
From the NASA Exoplanet Archive (ESO/ESPRESSO radial-velocity orbit)
Eccentricity
0.04
From the NASA Exoplanet Archive (ESO/ESPRESSO radial-velocity orbit)
Inclination
0.00 °
From the NASA Exoplanet Archive (ESO/ESPRESSO radial-velocity orbit)
Orbital period
2.3 days
From the NASA Exoplanet Archive (ESO/ESPRESSO radial-velocity orbit)
Perihelion
2,699,942 km
Computed from the orbital elements
Aphelion
2,924,938 km
Computed from the orbital elements
Mean orbital velocity
87.4 km/s
Computed from the orbital elements

Composition

Bulk composition
Presumed rocky (minimum mass ~0.26 Earth); never imaged.
Surface appearance
Appearance based on ESO/M. Kornmesser's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The surface shown is an artistic representation, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
9.9 S⊕ · 9.9× the sunlight Earth receives
Computed from Barnard's Star's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
483 K (210 °C)
Computed model value (no atmosphere assumed), the hottest of the four — not measured.

Discovery & history

Method
Radial-velocity detection (stellar wobble)
Name
Designated 'd' as the third planet found around Barnard's Star, following the IAU convention of lettering planets in discovery order starting at 'b'.

Part of the four-planet family established from ESO/ESPRESSO data in 2025 — the closest to the star, and the hottest.

Images

Never imaged — this world is known only from the tiny gravitational tug it exerts on its star (radial velocity). An artist's impression of the whole system is on the system view; the planet's own appearance is unknown.